464 citations · 889 across the 7 of their papers we have counts for
7 papers
Atmospheric neutrino flux at INO, South Pole and Pyhäsalmi
M. Sajjad Athar, M. Honda, T. Kajita +2
We present the calculation of the atmospheric neutrino fluxes for the neutrino experiments proposed at INO, South Pole and Pyhäsalmi. Neutrino fluxes have been obtained using ATMNC…
Calculation of atmospheric neutrino flux using the interaction model calibrated with atmospheric muon data
M. Honda, T. Kajita, K. Kasahara +2
Using the ``modified DPMJET-III'' model explained in the previous paper, we calculate the atmospheric neutrino flux. The calculation scheme is almost the same as HKKM04 \cite{HKKM2…
Microlensing optical depth towards the Galactic bulge from MOA observations during 2000 with Difference Image Analysis
T. Sumi, F. Abe, I. A. Bond +27
We analyze the data of the gravitational microlensing survey carried out by by the MOA group during 2000 towards the Galactic Bulge (GB). Our observations are designed to detect ef…
Atmospheric gamma-ray observation with the BETS detectorfor calibrating atmospheric neutrino flux calculations
K. Kasahara, E. Mochizuki, S. Torii +13
We observed atmospheric gamma-rays around 10 GeV at balloon altitudes (15~25 km) and at a mountain (2770 m a.s.l). The observed results were compared with Monte Carlo calculations…
Comparison of 3-Dimensional and 1-Dimensional Schemes in the calculation of Atmospheric Neutrinos
M. Honda, T. Kajita, K. Kasahara +1
A 3-dimensional calculation of atmospheric neutrinos flux is presented, and the results are compared with those of a 1-dimensional one. In this study, interaction and propagation o…
Uncertainty of the atmospheric neutrino fluxes
M. Honda
The uncertainty in the calculation of atmospheric neutrino fluxes is studied. The absolute value of atmospheric neutrino fluxes is sensitive to variation of the primary cosmic ray…
Comparison of Atmospheric Neutrino Flux Calculations at Low Energies
T. K. Gaisser, M. Honda, K. Kasahara +4
We compare several different calculations of the atmospheric neutrino flux in the energy range relevant for contained neutrino interactions, and we identify the major sources of di…